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Charged rotating AdS black hole and its thermodynamics in conformal gravity

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Abstract

We obtain the charged rotating black hole in conformal gravity. The metric is asymptotic to the (anti-)de Sitter spacetime. The contribution to the metric from the charges has a slower falloff than that in the Kerr-Newman AdS black hole. We analyse the global structure and obtain all the thermodynamical quantities including the mass, angular momentum, electric/magnetic charges and their thermodynamical conjugates. We verify that the first law of thermodynamics holds. We also obtain the new neutral rotating black holes that are beyond Einstein metrics. In contrast to the static ones, these rotating black holes have no parameters associated with the massive spin-2 hair.

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Authors and Affiliations

  1. Institute for Advanced Physics & Mathematics, Zhejiang University of Technology, Hangzhou, 310023, China

    Hai-Shan Liu

  2. Department of Physics, Beijing Normal University, Beijing, 100875, China

    H. Lü

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  1. Hai-Shan Liu
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  2. H. Lü
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Correspondence to Hai-Shan Liu.

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ArXiv ePrint: 1212.6264

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Liu, HS., Lü, H. Charged rotating AdS black hole and its thermodynamics in conformal gravity. J. High Energ. Phys. 2013, 139 (2013). https://doi.org/10.1007/JHEP02(2013)139

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